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C7H
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JeffMangum
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Detailed Information for C
7
H
Last Update:
JeffMangum
- 16 Dec 2005
Laboratory Measurements:
Travers, M. J., McCarthy, M. C., Gottlieb, C. A., and Thaddeus, P.,
Laboratory Detection of the C7H Radical
, 1996, ApJ, 465, L77
Molecular Structure and Constants:
Electronic Ground State Doublet Pi
Aeff = 769735(16) MHz (25.68 cm-1)
B = 875.48405(6) MHz
D x 10^6 = 11.280 (4) MHz
p + 2q = 1.574(11)
q = -.0164(2)
Doublet Pi 1/2 Rotational Constant Beff=874.4869(2) MHz Deffx10^6=10.04(2) (Travers et al. 1996)
Doublet Pi 3/2 Rotational Constant Beff=876.4812(2) MHz Deffx10^6=12.53(1) (Travers et al. 1996)
Dipole Moment 5.95 Debye (est.)
Astronomical Detection:
Guelin, M., Cernicharo, J., Travers, M. J., McCarthy, M. C., Gottlieb, C. A., Thaddeus, P., Ohishi, M., Saito, S., and Yamamoto, S.,
Detection of a New Linear Carbon Chain Radical: C7H
, 1997, A&A, 317, L1
. Five lines observed toward the evolved carbon star IRC+10216 indicate the molecule is four times less abundant than
C8H
and twenty times less abundant than
C5H
in the molecular shell surrounding the star. Typically, in the J=48.5 -> 47.5 transitions near 85 GHz, an integrated line intensity of 0.08(2) was observed in each of the lambda-doublet components with the IRAM 30m telescope.
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Topic revision: r1 - 2005-12-17,
JeffMangum
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